Single Degenerate Progenitors of Type Ia Supernovae

被引：0

作者：

Bours, Madelon ^{[1
]}

Toonen, Silvia ^{[1
]}

Nelemans, Gijs ^{[1
]}

机构：

[1] Radboud Univ Nijmegen, Dept Astrophys, IMAPP, Nijmegen, Netherlands

来源：

BINARY PATHS TO TYPE IA SUPERNOVAE EXPLOSIONS | 2013年 / 281期

关键词：

stars:; supernovae; white dwarfs; binaries:; close; symbiotic; accretion; WHITE-DWARFS; EVOLUTION; MATTER; RATES;

D O I：

10.1017/S1743921312015141

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

There is a general agreement that Type Ia supernovae correspond to the thermonuclear runaway of a white dwarf (WD) in a compact binary. The details of these progenitor systems are still unclear. Using the population synthesis code SeBa and several assumption for the WD retention efficiency, we estimate the delay times and supernova rates for the single degenerate scenario.

引用

页码：248 / 250

页数：3

共 10 条

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